Table 2
Results of the correlation analysis.
| Variables | Disp. | r(N) | Sign. |
|
|
|||
| Agn dominated quasars | |||
|
|
|||
| log SFR vs. Max velocity | 0.2 | 0.44(39) | 95% |
| SFR vs. Wings vel. offset | 0.2 | 0.40(39) | 95% |
| log SFR vs. (σ [OIII]–σ [OII]) | 0.2 | 0.45(33) | 95% |
|
|
|||
| SB dominated quasars | |||
|
|
|||
| log SFR vs. Max velocity | 0.5 | 0.23(86) | NO |
| log SFR vs. Wings offset | 0.5 | 0.11(86) | NO |
| log SFR vs. Δ VSIG [OIII] | 0.5 | 0.22(75) | NO |
Notes. Column 2: the variance of the intrinsic scatter. Column 3: the linear correlation coefficient between the dependent and independent variables (Pearson product-moment correlation coefficient). The maximum positive (negative) correlation is indicated by a correlation coefficient of 1 (−1). An absolute value between 0.4 and 0.7 could indicate moderate association. Column 4: significance of the linear correlation. A value of P less than 0.01 (0.05) imply a significant measurement at 1% (5%), id.e. there is 1% (5%) percentage chance that the finding is non-significant. N is the size of the sample.
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